A new code for radiation processes in high energy plasmas

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dc.creatorBelmont, R.
dc.creatorMalzac, J.
dc.creatorMarcowith, A.
dc.date2008-02-19
dc.date.accessioned2026-07-07T09:21:44Z
dc.date.available2026-07-07T09:21:44Z
dc.descriptionExtreme objects such as X-ray binaries, AGN, or $γ$-ray bursters harbor high energy plasmas whose properties are not well understood yet. Not only are they responsible of the hard X- and $γ$-ray emission we observe but also they have a strong influence on the main dynamics and energetics of these objects themselves. Here we present a new kinetic code that solves the evolution equations for particles and photons around compact objects. It produces spectra that will be compared with observations from Simbol-X to constrain the radiation and acceleration processes in these objects.
dc.descriptionPoster at the international workshop 'Simbol-X: the hard X-ray universe in focus' held in Bologna, 14-16 May 2007. To appear in Memorie della SAIt, 2 pages, 1 figure
dc.identifierhttps://arxiv.org/abs/0802.2661
dc.identifierhttp://arxiv.org/abs/0802.2661
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/155131
dc.subjectAstrophysics
dc.titleA new code for radiation processes in high energy plasmas
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